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Proteus - Geology, shape, and catastrophic destructionLeast-squares fits to the two available limb profiles of Proteus yield a sphericity close to unity; the visual irregularity is due to a degree of surface roughness comparable to that of Hyperion and the smaller icy satellites. A network of streaks that can be interpreted as tectonic troughs cuts the surface of Proteus, and is organized concentrically around either one of the two nearly-coincident Proteus-Neptune of Pharos axes of symmetry. If the streaks are tectonic, they may be due to tidal stresses generated by a past change in Proteus' equilibrium orientation. The streaks may also be disruptive-stress fractures.
Document ID
19930030910
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Croft, Steven K.
(Arizona Univ. Tucson, United States)
Date Acquired
August 16, 2013
Publication Date
October 1, 1992
Publication Information
Publication: Icarus
Volume: 99
Issue: 2
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
93A14907
Funding Number(s)
CONTRACT_GRANT: NAGW-2021
Distribution Limits
Public
Copyright
Other

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